The star formation rates of QSOs

dc.contributor.authorSymeonidis, Myrto
dc.contributor.authorMaddox, Natasha
dc.contributor.authorJarvis, Matthew J.
dc.date.accessioned2022-08-03T13:09:51Z
dc.date.available2022-08-03T13:09:51Z
dc.date.issued2022
dc.description.abstractWe examine the far-IR properties of a sample of 5391 optically selected QSOs in the 0.5 < z < 2.65 redshift range down to log [νLν,2500(erg/s)] > 44.7, using SPIRE data from Herschel-ATLAS. We split the sample in a grid of 74 luminosity-redshift bins and compute the average optical–infrared spectral energy distribution (SED) in each bin. By normalising an intrinsic AGN template to the AGN optical power (at 5100˚A) we decompose the total infrared emission (LIR; 8—1000µm) into an AGN (LIR,AGN) and star-forming component (LIR,SF). We find that the AGN contribution to LIR increases as a function of AGN power which manifests as a reduction of the ‘far-IR bump’ in the average QSO SEDs. We note that LIR,SF does not correlate with AGN power; the mean star formation rates (SFRs) of AGN host galaxies are a function of redshift only and they range from ∼6 M⊙/yr at z ∼ 0 to a plateau of . 200 M⊙/yr at z ∼ 2.6.en_US
dc.identifier.citationSymeonidis, M. et al. (2022). The star formation rates of QSOs. Monthly Notices of the Royal Astronomical Society, 514(3), 4450-4464. 10.1093/mnras/stac1359en_US
dc.identifier.issn1365-2966
dc.identifier.uri10.1093/mnras/stac1359
dc.identifier.urihttp://hdl.handle.net/10566/7661
dc.language.isoenen_US
dc.publisherRoyal Astronomical Societyen_US
dc.subjectAstrophysicsen_US
dc.subjectRedshiften_US
dc.subjectNuclearen_US
dc.subjectAGN poweren_US
dc.titleThe star formation rates of QSOsen_US
dc.typeArticleen_US

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